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Background coincidences

The off-energy electron background disturbs the VSAT data in many ways, as will be discussed in section 4.1 the coincidence of two off-energy electrons can trigger a Bhabha event. This ``false Bhabha'' rate normally stays below 30% of the number of Bhabha triggers, but can at times go above 50% (Fig. 3.6). Most of the false Bhabhas can be removed with narrow cuts due to the well confined properties of a true Bhabha event. The remaining background can be quantized by a linear combination of four different measurements [16]:

Ecut/($\displaystyle {\frac{S_1\cdot S_2}{SE_1 SE_2}}$ - 1)        $\displaystyle {\frac{SE_1 \cdot SE_2}{\Delta T}}$        Bsoft - Bhard        FBscal

Here Ecut is the number of events cut away by the Bhabha energy cut, S and SE the number of downscaled off-energy electron triggers with and without the energy cut. The duration of the measured data is given by $ \Delta$T and Bsoft - Bhard is the difference between the normal Bhabha sample and one with especially hard background cuts. Finally the FBscal is the online delayed Bhabha scaler (taken as the coincidence of two opposite hits separated by four bunch crossings), which only is usable in cases of bad statistics.


A $ \gamma$$ \gamma$-event is triggered by cuts on the hadronic system in the DELPHI detector (section 5.1). If an off-energy electron coincides with the hadronic trigger, it can result in any of the following VSAT $ \gamma$$ \gamma$-event:

The most troublesome background for this analysis is the second , as the confinement of the off-energy background is mixed up with the spread of true $ \gamma$$ \gamma$-events. The other two background triggers could in principle be completely removed by strong cuts, without too much loss of the signal. This is not possible for second type and the size of the background has to be estimated in order to make an efficiency calculation.


next up previous contents
Next: Probabilities Up: Off-Energy Background Previous: Trigger Rate
Andreas Nygren
2001-10-24